Radio halos in a mass-selected sample of 75 galaxy clusters - I. Sample selection and data analysis

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Volume 647 (March 2021)

A&A, 647 (2021) A50

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Table 1.

Total sample clusters properties.

Cluster name	RA	Dec	z	M₅₀₀	R₅₀₀	Radio	P_1.4 GHz
				(10¹⁴ M_⊙)	(kpc)	info	(10²⁴ W Hz⁻¹)
A1437	12 00 22.3	+03 20 33.9	0.134		1200	No RH^( * )	–
A2345	21 27 06.8	−12 07 56.0	0.176		1190	UL⁽⁴⁾	< 0.38
A2104	15 40 08.2	−03 18 23.0	0.153		1200	UL^( * )	< 0.24
Zwcl 2120.1+2256	21 22 27.1	+23 11 50.3	0.143		1200	RH(c)^( * )	–
RXC J0616.3−2156	06 16 22.8	−21 56 43.4	0.171		1200	UL^( * )	< 0.25
A1413	11 55 18.9	+23 24 31.0	0.143		1220	MH⁽⁵⁾	–
A1576	12 37 59.0	+63 11 26.0	0.302		1160	UL⁽⁶⁾	< 0.64
A2697	00 03 11.8	−06 05 10.0	0.232		1190	UL⁽²⁾	< 0.41
Z5247	12 33 56.1	+09 50 28.0	0.229		1190	RH(c)⁽⁷⁾	–
Zwcl 0104.9+5350	01 07 54.0	+54 06 00.0	0.107		1240	RH⁽⁸⁾	1.62 ± 0.15
RXC J0142.0+2131	01 42 02.6	+21 31 19.0	0.280		1170	RH^(40),US(c)	0.42 ± 0.01
A1423	11 57 22.5	+33 39 18.0	0.214		1200	UL⁽²⁾	< 0.38
ZwCl 1028.8+1419	10 31 28.2	+14 03 34.0	0.310		1160	No RH^( * )	–
A3041	02 41 22.1	−28 38 13.0	0.230		1190	RH(c)^( * )	–
RXC J2051.1+0216	20 51 08.0	+02 15 55.0	0.320		1150	UL^( * )	< 0.73
A2472	22 41 50.6	+17 31 43.0	0.310		1160	UL^( * )	< 1.0
A2895	01 18 11.1	−26 58 23.0	0.230		1190	UL^( * )	< 0.5
RXC J1314.4–2515	13 14 28.0	−25 15 41.0	0.244		1190	RH^(1), US(c)	0.68 ± 0.24
A2537	23 08 23.2	−02 11 31.0	0.297		1170	UL⁽²⁾	< 0.45
A68	00 37 05.3	+09 09 11.0	0.255		1190	UL⁽⁷⁾	< 0.42
A56	00 33 50.4	−07 47 28.0	0.300		1170	UL^( * )	< 1.2
A1682	13 06 49.7	+46 32 59.0	0.226		1200	RH(c)⁽²⁾	–
A1132	10 58 19.6	+56 46 56.0	0.134		1240	RH^(27),US	0.16 ± 0.08
RXJ1720.1+2638	17 20 10.1	+26 37 29.5	0.164		1240	MH+USSRH^(9, 40)	–
A781	09 20 23.2	+30 26 15.0	0.295		1180	UL⁽²⁾	< 0.36
A384	02 48 13.9	−02 16 32.0	0.240		1210	UL^( * )	< 0.74
A2218	16 35 51.6	+66 12 39.0	0.171		1240	RH⁽³⁾	0.44 ± 0.10
A3411	08 41 55.6	−17 29 35.7	0.169		1250	RH⁽¹⁰⁾	0.27 ± 0.1
Zwcl 0634.1+4750	06 38 02.5	+47 47 23.8	0.174		1250	RH⁽²⁵⁾	0.31 ± 0.02
RXC J1322.8+3138	13 22 48.8	+31 39 17.0	0.310		1190	No RH^( * )	–
A3888	22 34 26.8	−37 44 19.1	0.151		1260	RH^( * ,33)	1.90 ± 0.20
A3088	03 07 04.1	−28 40 14.0	0.254		1220	UL⁽²⁾	< 0.43
A220	01 37 19.5	+07 56 16.0	0.330		1190	UL^( * )	< 0.97
A2667	23 51 40.7	−26 05 01.0	0.226		1240	MH⁽²⁸⁾	–
A521	04 54 09.1	−10 14 19.0	0.248		1240	RH^(11),US	1.45 ± 0.13
A2355	21 35 22.5	+01 23 26.0	0.230		1240	UL^( * )	< 0.83
A2631	23 37 40.6	+00 16 36.0	0.278		1230	UL⁽²⁾	< 0.41
A1914	14 26 03.0	+37 49 32.0	0.171		1280	No RH⁽³⁵⁾	–
RXC J1504.1–0248	15 04 07.7	−02 48 18.0	0.215		1330	MH⁽¹³⁾	–
A1733	13 27 03.7	+02 12 15.0	0.260		1240	UL^( * )	< 0.53
A520	04 54 19.0	+02 56 49.0	0.203		1270	RH⁽¹⁴⁾	2.45 ± 0.18
A478	04 13 20.7	+10 28 35.0	0.088		1320	MH^(15, 40)	–
A773	09 17 59.4	+51 42 23.0	0.217		1260	RH⁽¹⁴⁾	1.48 ± 0.16
PSZ1 G019.12+3123	16 36 29.4	+03 08 51.0	0.280		1230	UL^( * )	< 0.63
PSZ1 G139.61+24.20	06 22 13.9	+74 41 39.0	0.270		1210	MH+USSRH^(28, 29)	–
A1351	11 42 30.8	+58 32 20.0	0.322		1210	RH⁽¹⁶⁾	9.30 ± 1.5
A115	00 55 59.5	+26 19 14.0	0.197		1280	No RH⁽¹⁴⁾	–
A402	02 57 41.1	−22 09 18.0	0.320		1220	MH (c)^( * )	–
A1451	12 03 16.2	−21 32 12.7	0.199		1290	RH⁽²⁵⁾	0.64 ± 0.07
RXCJ 0510.7–0801	05 10 47.9	−08 01 06	0.220		1280	No RH⁽⁷⁾	–
PSZ1 G205.07–6294	02 46 27.5	−20 32 5.29	0.310		1240	No RH^(p)	–
A2261	17 22 17.1	+32 08 02.0	0.224		1280	RH^{(30, 34),US(c)}	0.68 ± 0.07
RXCJ2003.5–2323	20 03 30.4	−23 23 05.0	0.317		1240	RH⁽¹⁾	10.71 ± 1.73
A2552	23 11 26.9	+03 35 19.0	0.300		1250	RH(c)⁽⁷⁾	–
MACS J2135-010	21 35 12.1	−01 02 58.0	0.330		1240	UL^( * )	< 1.17
A3444	10 23 50.8	−27 15 31.0	0.254		1270	MH^(7, 28)	–
S780	14 59 29.3	−18 11 13.0	0.236		1290	MH^(7, 28)	–
A1443	12 01 27.7	+23 05 18.0	0.270		1270	RH⁽³¹⁾	0.91 ± 0.04
A2204	16 32 45.7	+05 34 43.0	0.151		1340	MH⁽¹⁵⁾	–
A1758a	13 32 32.1	+50 30 37.0	0.280		1280	RH⁽¹⁷⁾	5.75 ± 0.98
A209	01 31 53.0	−13 36 34.0	0.206		1330	RH⁽¹⁾	1.99 ± 0.21
A665	08 30 45.2	+65 52 55.0	0.182		1340	RH⁽³⁾	2.51 ± 0.21
A1763	13 35 17.2	+40 59 58.0	0.228		1320	No RH⁽²⁾	–
RXC J1514.9–1523	15 14 58.0	−15 23 10.0	0.223		1330	RH^(18),US(c)	2.39 ± 0.70
A1835	14 01 02.3	+02 52 48.0	0.253		1320	MH⁽¹⁹⁾	-
A2142	15 58 16.1	+27 13 29.0	0.089		1420	RH^{(24, 32),US(c)}	0.19 ± 0.06
A1689	13 11 29.5	−01 20 17.0	0.183		1380	RH⁽²⁰⁾	0.95 ± 0.28
A1300	11 31 56.3	−19 55 37.0	0.308		1310	RH^(21),US(c)	3.80 ± 1.43
A2813	00 43 27.4	−20 37 27.0	0.290		1340	UL^( * )	< 1.4
A2390	21 53 34.6	+17 40 11.0	0.234		1380	No RH⁽³⁴⁾	–
A2744	00 14 18.8	−30 23 00.0	0.307		1350	RH⁽¹⁴⁾	17.40 ± 0.90
A2219	16 40 21.1	+46 41 16.0	0.228		1450	RH⁽¹²⁾	5.63 ± 0.80
PSZ1 G171.96-40.64	03 12 57.4	+08 22 10.0	0.270		1440	RH^(22),US(c)	4.90 ± 1.35
A697	08 42 53.3	+36 20 12.0	0.282		1190	RH^(2),US	1.51 ± 0.14
A2163	16 15 46.9	−06 08 45.0	0.203		1680	RH⁽²³⁾	22.90 ± 1.16

Notes. RH = Radio Halo, MH = Mini Halo, UL = Upper Limit, US = Ultra Steep, c = candidate. P_1.4 GHz = k-corrected radio power at 1.4 GHz.

References. ^( * )This paper, ⁽¹⁾Venturi et al. (2007), ⁽²⁾Venturi et al. (2008), ⁽³⁾Giovannini & Feretti (2000), ⁽⁴⁾Bonafede et al. (2017), ⁽⁵⁾Govoni et al. (2009), ⁽⁶⁾Kale et al. (2013), ⁽⁷⁾Kale et al. (2015), ⁽⁸⁾van Weeren et al. (2011), ⁽⁹⁾Giacintucci et al. (2014a), ⁽¹⁰⁾van Weeren et al. (2013), ⁽¹¹⁾Brunetti et al. (2008), ⁽¹²⁾Bacchi et al. (2003), ⁽¹³⁾Giacintucci et al. (2011a), ⁽¹⁴⁾Govoni et al. (2001), ⁽¹⁵⁾Giacintucci et al. (2014b), ⁽¹⁶⁾Giacintucci & Venturi (2009), ⁽¹⁷⁾Giovannini et al. (2006), ⁽¹⁸⁾Giacintucci et al. (2011b), ⁽¹⁹⁾Murgia et al. (2009), ⁽²⁰⁾Vacca et al. (2011), ⁽²¹⁾Reid et al. (1999), ⁽²²⁾Giacintucci et al. (2013), ⁽²³⁾Feretti et al. (2001), ⁽²⁴⁾Farnsworth et al. (2013), ⁽²⁵⁾Cuciti et al. (2018), ⁽²⁶⁾Cassano et al. (2013), ⁽²⁷⁾Wilber et al. (2018), ⁽²⁸⁾Giacintucci et al. (2017), ⁽²⁹⁾Savini et al. (2018), ⁽³⁰⁾Sommer et al. (2017), ⁽³¹⁾Bonafede et al. (2015), ⁽³²⁾Venturi et al. (2017), ⁽³³⁾Shakouri et al. (2016a), ⁽³⁴⁾Savini et al. (2019), ⁽³⁵⁾Mandal et al. (2019), ^(p)Ferrari et al. (priv. comm.).

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